Chapter 7: Radiation and Matter Flashcards

1
Q

Interaction btwn Radiation and Matter

(Hamiltonian)

A
  • Decompose into interacting and non-interacting parts
  • NOTE: Assumes Coulomb gauge [A,p]=0
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2
Q

Interaction btwn Radiation and Matter

(Hilbert Space)

A

Only Hint acts on both spaces

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3
Q

Time-Dependent Perturbation Theory

(Hamiltonian)

A
  • H0 is time-independent and complete eigenbasis is known
  • H’(t) is small
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4
Q

Interaction Picture

(Overview)

A
  • Intermediary picture between Schrödinger and Heisenberg
  • Expectation values are invariant
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5
Q

Dirac Time-Evolution Operators

A

Expand UD(t) to get approximations

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6
Q

Interaction Picture

(Wavefunction)

A
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7
Q

Interaction Picture

(Operators)

A
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8
Q

Interaction Picture

(Schrödinger Equation)

A
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9
Q

Interaction Picture

(Summary)

A
  • States evolve under interaction Hamiltonian
  • Operators evolve under non-interacting Hamiltonian
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10
Q

Fermi’s Golden Rule

(Transition Probability)

A

Gives probability for the transition between two states due to external excitation

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11
Q

Fermi’s Golden Rule

(Rate Equation)

A
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12
Q

Fermi’s Golden Rule

(Rate Equation [Multiple Final States])

A

ρ(Ei) ≡ density of state at Ei

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13
Q

Hydrogen Atom in Radiation Field

(Assumptions)

A
  • Hailtonian: H = H0 + H’= (Hpart + Hem) + Hint
  • Initial state:
    • | i > ≡ | a > | n<em>kλ</em> >
    • Ei = Ea + (hbar) ωn
  • Final state:
    • | f > ≡ | b > | n<em>kλ</em> + 1 >
    • Ef = Eb + (hbar) ω(n+1) = Ei
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14
Q

Hydrogen Atom in Radiation Field

(Take-Away)

A
  • δ(EiEf) gives that emitted photon must have energy equal to energy difference of final and initial energies
  • Transition rate yield expressions for stimulated/sponstaneous emission and stimulated absorptions
    • n = 0 → spontaneous emission
    • n > 0 → stimulated emission/absorption
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15
Q

Hydrogen Atom in Radiation Field

(Notes)

A
  • ω3/c2 ∈ field
  • rab ∈ atom
  • fine structure constant α ≡ coupling strength between matter and radiation
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16
Q

Hydrogen Atom in Radiation Field

(Selection Rules)

A
  • Evaluating dipole overlap term r<em>ab </em>leads to selection rules
  • Matrix element vanishes unless ∆l = ±1, ∆m = ±1, 0